Wow! 1st Interstellar Asteroid Is a Spinning Space Cigar

When astronomers using the Pan-STARRS1 telescope in Hawaii spotted a mysterious object dashing through our solar system on Oct. 19, they immediately knew it was something special. 

Traveling at high speed and originating from interstellar space, this object was originally thought to be an ancient comet, but observations revealed it was, in fact, an asteroid from another star system. 

"For decades we’ve theorized that such interstellar objects are out there, and now — for the first time — we have direct evidence they exist," Thomas Zurbuchen, associate administrator for NASA’s Science Mission Directorate at the agency's headquarters in Washington, D.C., said in a statement. [Solar System Explained from the Inside Out (Infographic)]

"This history-making discovery is opening a new window to study formation of solar systems beyond our own," he added.

This artist’s illustration shows the first interstellar asteroid, ‘Oumuamua. This unique object was discovered on Oct. 19, 2017 by the Pan-STARRS 1 telescope in Hawaii. Subsequent observations from ESO’s Very Large Telescope in Chile and other observatories around the world show that ‘Oumuamua seems to be a dark red highly elongated metallic or rocky object, about 1,300 feet (400 meters) long, and is unlike anything normally found in the solar system. (Image credit: M. Kornmesser/ESO)

Astronomers have determined that the mysterious object — which has been named 'Oumuamua and given the official scientific designation 1I/2017 U1 — looped around the sun on Sept. 9 and made its closest pass by Earth on Oct. 14. 'Oumuamua (whose name means "a messenger from afar arriving first" in Hawaiian) is now about 124 million miles (200 million kilometers) from Earth and is zooming away from us at about 85,700 mph (137,900 km/h) relative to the sun, NASA officials said.

Researchers scrambled to get some good looks of the interstellar interloper, which have revealed that this object is very special indeed. In fact, it's like nothing we’ve ever seen before.

"It's a really rare object," astronomer Ralf Kotulla, of the University of Wisconsin-Madison, said in a different statement.

This very deep combined image shows the interstellar asteroid ‘Oumuamua at the center of the picture. It is surrounded by the trails of faint stars that are smeared as the telescopes tracked the moving asteroid. This image was created by combining multiple images from ESO’s Very Large Telescope as well as the Gemini South Telescope. The object appears to be a point source, with no surrounding dust. (Image credit: K. Meech et al./ESO)

With colleagues from UCLA and the National Optical Astronomy Observatory (NOAO), Kotulla's team captured some of the first images of U1 using the 11.5-foot (3.5 meters) WIYN Telescope on Kitt Peak in Arizona. These first images confirmed that the object doesn't have a coma — the cloud of dust and gas that fizzes from a comet as it approaches the sun — and is therefore an irregularly shaped asteroid.

Now, in a study published today (Nov. 20) in the journal Nature, astronomers using the European Southern Observatory's (ESO) Very Large Telescope (VLT) in Chile describe the strange characteristics of U1.

The VLT’s FORS instrument was able to make very precise spectroscopic measurements of 'Oumuamua's brightness and color. By combining the VLT observations with those made by other telescopes, astronomers found that 'Oumuamua's brightness varies by a factor of 10 as it spins on its axis every 7.3 hours.

"This unusually large variation in brightness means that the object is highly elongated: about 10 times as long as it is wide, with a complex, convoluted shape," astronomer Karen Meech, of the Institute for Astronomy in Hawaii, said in another statement, this one put out by ESO. "We also found that it has a dark red color, similar to objects in the outer solar system, and confirmed that it is completely inert, without the faintest hint of dust around it."

This graph shows how the interstellar asteroid ‘Oumuamua varied in brightness during three days in October 2017. The large range of brightness — about a factor of 10 (2.5 magnitudes) — is due to the very elongated shape of this unique object, which rotates every 7.3 hours. The different-colored dots represent measurements through different filters, covering the visible and near-infrared part of the spectrum. The dotted line shows the light curve expected if ‘Oumuamua were an ellipsoid with a 1:10 aspect ratio; the deviations from this line are probably due to irregularities in the object's shape or surface albedo. (Image credit: K. Meech et al./ESO)

'Oumuamua is thought to be at least 1,300 feet (400 m) long, rocky (with some metal perhaps mixed in), relatively dense and shaped like a cigar, researchers said. It likely acquired its ruddy hue after being bombarded by high-energy cosmic rays for the millions of years it's been drifting through interstellar space, team members added. 

Using the NASA/European Space Agency Hubble Space Telescope and NASA's Spitzer space telescope, astronomers continue to study 'Oumuamua as it heads toward the outer solar system, in an attempt to learn more about this strange object.

"We are continuing to observe this unique object, and we hope to more accurately pin down where it came from and where it is going next on its tour of the galaxy," observation team member Olivier Hainaut, from ESO in Garching, Germany, said in the ESO statement. "And now that we have found the first interstellar rock, we are getting ready for the next ones!"

Astronomers estimate that such interstellar visitors shoot though the inner solar system about once a year, but only recently, with the incredibly powerful optics of telescopes like Pan-STARRS1, have they been able to detect these very faint objects.

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Media Relations Specialist, NASA's Jet Propulsion Laboratory

Ian O'Neill is a media relations specialist at NASA's Jet Propulsion Laboratory (JPL) in Southern California. Prior to joining JPL, he served as editor for the Astronomical Society of the Pacific‘s Mercury magazine and Mercury Online and contributed articles to a number of other publications, including,, Live Science,, Scientific American. Ian holds a Ph.D in solar physics and a master's degree in planetary and space physics.